Which show that, in the weak field regime, the correction in the
\(y\) -orientation is three times greater than in the \(x\) -orientation. For the
example of a Casimir device resting at the equator of a spinning neutron star,
considering \(M\simeq 1.4M_{\odot }\) , \(r\simeq 10^{4}\operatorname{m}\)  and \(\Omega \simeq 190\operatorname{rad}/\operatorname{s}\) , the reference [1]} determines \(x=2.3\times 10^{-5}\) .
